Ice in the northern lowlands and southern highlands of Mars and its enrichment beneath the Elysium Lavas

Details Ice in the northern lowlands and southern highlands of Mars and its enrichment beneath the Elysium Lavas Ice in the northern lowlands and southern highlands of Mars and its enrichment beneath the Elysium Lavas

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992msat.work...30c&link_type=abstract

In Lunar and Planetary Inst., Workshop on the Martian Surface and Atmosphere Through Time p 30-31 (SEE N92-28988 19-91)

Mathematics

Logic

Ejecta, Geomorphology, Ice, Mars Craters, Mars Surface, Moisture Content, Planetary Geology, Highlands, Lava, Mobility

Scientific paper

The simultaneously examination of ejecta mobility, crater morphology, and surface features has enabled several conclusions to be drawn regarding the location of subsurface ice in the region. The ice distribution is shown to be highly dependent upon latitude and geological situation; in particular, pronounced differences in the distribution between the highland and lowlands are seen, and concentrations of ice were detected beneath the Elysium lavas.

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